The stellar mass - halo mass relation (SHMR) obtained from model M2
is shown in Figure REF . For comparison, the result
for the total central sample, cG, obtained using model M1 is shown
as green points. As references, the SHMR derived by
various methods in the literature, including galaxy group
catalog [1]}, abundance matching
[2]}, [3]},
conditional luminosity function [4]} and
weak lensing [5]} are presented. Our result
for the total sample is in good agreement with previous results,
indicating that our method is reliable.
In general, the halo mass increases with stellar mass.
And there is a pivot halo mass around \(10^{12}\, h^{-1}{\rm M_\odot }\) ,
above and below which the SHMR have different slopes.
